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http://hdl.handle.net/2248/6735
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DC Field | Value | Language |
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dc.contributor.author | Tandon, S. N | - |
dc.contributor.author | Ghosh, S. K | - |
dc.contributor.author | Hutchings, J | - |
dc.contributor.author | Stalin, C. S | - |
dc.contributor.author | Subramaniam, A | - |
dc.date.accessioned | 2020-11-10T02:32:31Z | - |
dc.date.available | 2020-11-10T02:32:31Z | - |
dc.date.issued | 2017-08 | - |
dc.identifier.citation | Current Science, Vol. 113, No. 4, pp. 583 - 586 | en_US |
dc.identifier.issn | 0011-3891 | - |
dc.identifier.uri | http://prints.iiap.res.in/handle/2248/6735 | - |
dc.description | Open Access © Current Science Association http://www.currentscience.ac.in/Volumes/113/04/0583.pdf | en_US |
dc.description.abstract | The AstroSat satellite is designed for multiwavelength astronomy for observations covering a spectral range from soft and hard X-rays to the ultraviolet. The Ultraviolet Imaging Telescope (UVIT) is the only non-X-ray telescope on AstroSat and it provides the long lever arm to the multi-wavelength observations. In addition to the simultaneous multiwavelength studies in coordination with the X-ray telescopes on-board AstroSat, UVIT is used to study a large variety of objects with arcsecond-level spatial resolution. During the first year of observations, UVIT has obtained images in many filter bands in the wavelength range 130–300 nm over a field of ~28, which are being used to study a variety of hot stars, nebulae, stellar clusters and galaxies. | en_US |
dc.language.iso | en | en_US |
dc.publisher | Current Science Association | en_US |
dc.subject | Multi-wavelength astronomy | en_US |
dc.subject | Ultraviolet Imaging Telescope | en_US |
dc.subject | X-ray telescope | en_US |
dc.title | Ultraviolet Imaging Telescope on AstroSat | en_US |
dc.type | Article | en_US |
Appears in Collections: | IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
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Ultraviolet Imaging Telescope on A.pdf | 2.69 MB | Adobe PDF | View/Open |
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